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Bryan A. Baum1
Ping Yang2, Andrew Heymsfield3
1 NASA Langley Research Center, Hampton, VA 2 Texas A&M University, College Station, TX 3 National Center for Atmospheric Research, Boulder, CO
Goal: Provide ice cloud bulk scattering models that are developed consistently for suite of multispectral and hyperspectral instruments
Hyperspectral/Multispectral Ice Cloud Microphysical and Optical Models
Hyperspectral/Multispectral Ice Cloud Microphysical and Optical Models
5th Workshop on Hyperspectral Science June 7-9, 2005
Bulk Scattering ModelsBulk Scattering Models
Operational satellite-based cloud retrievals require the ability to simulate realistic ice cloud radiances quickly
Simulations require bulk scattering parameters such as
single-scattering albedoscattering phase function or asymmetry factorextinction efficiency or scattering/absorption cross sections
Scattering parameters in turn are based on the
cloud phase (ice, water, or mixed)particle size distributionparticle habit distributionwavelength(s)
Have libraries of scattering properties from Ping Yang & colleagues
Library of SWIR to Far-IR Scattering Properties100 to 3250 cm-1
Library of SWIR to Far-IR Scattering Properties100 to 3250 cm-1
Library of ice particle scattering properties include
Hexagonal platesSolid and hollow columnsAggregatesDroxtals3D bullet rosettes
45 size bins ranging from 2 to 9500 m
Spectral range: 100 to 3250 cm-1 at 1-cm-1 resolution
Properties for each habit/size bin include volume, projected area, maximum dimension, single-scattering albedo, asymmetry factor,and extinction efficiency
* Yang, P., H. Wei, H. L Huang, B. A. Baum, Y. X. Hu, M. I. Mishchenko, and Q. Fu, Scattering and absorption property database of various nonspherical ice particles in the infrared and far-infrared spectral region. In press, Applied Optics.
Particle Size Distributions Particle Size Distributions
Gamma size distribution* has the form:
N(D) = NoDe-D
where D = max diameter
No = intercept
= dispersion
= slope
The intercept, slope, and dispersion values are derived for each PSD by matching three moments (specifically, the 1st, 2nd, and 6th moments)
Note: when = 0, the PSD reduces to an exponential distribution
*Heymsfield et al., Observations and parameterizations of particle size distributions in deep tropical cirrus and stratiform precipitating clouds: Results from in situ observations in TRMM field campaigns. J. Atmos. Sci., 59, 3457-3491, 2002.
Field Campaign InformationField Campaign Information
Field Campaign
Location Instruments Number of PSDs
FIRE-1 (1986) Madison, WI 2D-C, 2D-P 246
FIRE-II (1991) Coffeyville, KS Replicator 22
ARM-IOP (2000) Lamont, OK 2D-C, 2D-P, CPI 390
TRMM KWAJEX (1999)
Kwajalein, Marshall Islands
2D-C, HVPS, CPI 418
CRYSTAL-FACE (2002)
Off coast of Nicaragua
2D-C, VIPS 41
Probe size ranges are: 2D-C, 40-1000 m; 2D-P, 200-6400 m; HVPS (High Volume Precipitation Spectrometer), 200–6100 m; CPI (Cloud Particle Imager), 20-2000 m; Replicator, 10-800 m; VIPS (Video Ice Particle Sampler): 20-200 m.
Replicator Ice Crystal Profiles from FIRE Cirrus II CampaignReplicator Ice Crystal Profiles from FIRE Cirrus II Campaign
Particle Size DistributionsFrom Gamma Fits
Particle Size DistributionsFrom Gamma Fits
Midlatitude cirrus characteristics
• Size sorting more pronounced
• Small crystals at cloud top
• More often find pristine particles
Tropical cirrus anvil characteristics
Form in an environment having much higher vertical velocities
• Size sorting is not as well pronounced
• Large crystals often present at cloud top
• Crystals may approach cm in size.
• Habits tend to be more complex
• Note that CRYSTAL distributions tend to be the narrowest overall
Ice Particle Habit DistributionIce Particle Habit Distribution
At this point, we have- ice particle scattering library- wealth of microphysical data for ice clouds (1117 PSDs)
Next issue: develop a ice particle habit distribution that makes sense
Note: each idealized ice particle has a prescribed volume, and hence mass
Compare IWC and Dm computed from integrating over the habit and size distributions to those values estimated from techniques developed by Heymsfield and colleagues from analyses of their in situ data
Guidelines
4 size domains defined by particle maximum length
Droxtals: used only for smallest particles
Aggregates: only for particles > 1000 m
Plates: used only for particles of intermediate size
Ice Particle Habit Percentages Based on Comparison of Calculated to In-situ Dm and IWC
Ice Particle Habit Percentages Based on Comparison of Calculated to In-situ Dm and IWC
Proposed ice particlehabit mixture
Max length < 60 m100% droxtals 60 m < Max length < 1000 m 15% bullet rosettes 35% hexagonal plates 50% solid columns 1000 m < Max length < 2500 m45% solid columns45% hollow columns10% aggregates
Max length > 2500 m97% bullet rosettes 3% aggregates
Small Particle Sensitivity StudySmall Particle Sensitivity Study
Note that CRYSTAL distributions tend to be the narrowest overall
For all 41 CRYSTAL size distributions, increase the number of particles with Dmax < 20 m by a factor of 100 or 1000
For building look-up tables for operational retrievals, want discrete set of models that are evenly spaced in effective diameter
Development of Discrete Set of ModelsDevelopment of Discrete Set of Models
Bulk Scattering ModelsAvailable for Multiple Instruments
Bulk Scattering ModelsAvailable for Multiple Instruments
Provide bulk properties (mean and std. dev.) evenly spaced in Deff from 10 to 180 m for
asymmetry factor phase function
single-scattering albedo extinction efficiency & cross sections
IWC Dm
Models available at http://www.ssec.wisc.edu/~baum for
IR Spectral Models (100 to 3250 cm-1)
MODIS AVHRR AATSR MISR
VIRS MAS (MODIS Airborne Simulator)
ABI (Advanced Baseline Imager) POLDER (Polarization)
SEVIRI (Spinning Enhanced Visible InfraRed Imager)